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Record W2150429435 · doi:10.1093/mnras/stv2141

Constraints on the richness–mass relation and the optical-SZE positional offset distribution for SZE-selected clusters

2015· article· en· W2150429435 on OpenAlexaff
A. Saro, S. Bocquet, Eduardo Rozo, B. A. Benson, J. J. Mohr, E. S. Rykoff, M. Soares-Santos, L. E. Bleem, Scott Dodelson, P. Melchior, F. Sobreira, V. Upadhyay, J. Weller, T. M. C. Abbott, F. B. Abdalla, S. Allam, R. Armstrong, M. Banerji, A. H. Bauer, Matthew Bayliss, A. Benoit-Lévy, G. M. Bernstein, E. Bertin, M. Brodwin, D. Brooks, E. Buckley‐Geer, D. L. Burke, J. E. Carlstrom, R. Capasso, D. Capozzi, A. Carnero Rosell, M. Carrasco Kind, I. Chiu, R. Covarrubias, T. M. Crawford, M. Crocce, C. B. D’Andrea, L. N. da Costa, D. L. DePoy, S. Desai, T. de Haan, H. T. Diehl, J. P. Dietrich, P. Doel, C. E. Cunha, T. F. Eifler, A. E. Evrard, A. Fausti Neto, E. Fernández, B. Flaugher, P. Fosalba, J. Frieman, C. Gangkofner, E. Gaztañaga, D. W. Gerdes, D. Gruen, R. A. Gruendl, N. Gupta, C. Hennig, W. L. Holzapfel, K. Honscheid, Bhuvnesh Jain, D. J. James, K. Kuehn, N. Kuropatkin, O. Lahav, T. S. Li, H. Lin, M. A. G. Maia, M. March, J. L. Marshall, Paul Martini, M. McDonald, C. J. Miller, R. Miquel, B. Nord, R. L. C. Ogando, C. L. Reichardt, A. K. Romer, A. Roodman, M. Šako, E. Sánchez, M. Schubnell, I. Sevilla-Noarbe, R. C. Smith, B. Stalder, A. A. Stark, V. Strazzullo, E. Suchyta, M. E. C. Swanson, G. Tarlé, J. Thaler, D. Thomas, D. L. Tucker, V. Vikram, Anja von der Linden, A. R. Walker, Risa H. Wechsler, W. C. Wester, A. Zenteno, K. E. Ziegler

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2015
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsMcGill University
FundersSLAC National Accelerator LaboratoryNational Science FoundationFermilabConselho Nacional de Desenvolvimento Científico e TecnológicoUniversity College LondonDanmarks GrundforskningsfondDeutsche ForschungsgemeinschaftArgonne National LaboratoryEuropean Regional Development FundSmithsonian InstitutionU.S. Department of EnergyEuropean CommissionScience and Technology Facilities CouncilOhio State UniversityNational Research FoundationUniversity of PortsmouthUniversity of ChicagoIntegrated Electronics Engineering Center, Binghamton UniversityUniversity of Illinois at Urbana-ChampaignLawrence Berkeley National LaboratoryUniversity of PennsylvaniaFinanciadora de Estudos e ProjetosGordon and Betty Moore FoundationUniversity of SussexMinistério da Ciência e Tecnologia
KeywordsPhysicsAstrophysicsGalaxy clusterCluster (spacecraft)LambdaPopulationCosmic microwave backgroundCluster samplingSouth Pole TelescopeGalaxyOptics

Abstract

fetched live from OpenAlex

We cross-match galaxy cluster candidates selected via their Sunyaev–Zel'dovich effect (SZE) signatures in 129.1 deg2 of the South Pole Telescope 2500d SPT-SZ survey with optically identified clusters selected from the Dark Energy Survey science verification data. We identify 25 clusters between 0.1 ≲ z ≲ 0.8 in the union of the SPT-SZ and redMaPPer (RM) samples. RM is an optical cluster finding algorithm that also returns a richness estimate for each cluster. We model the richness λ-mass relation with the following function 〈ln λ|M500〉 ∝ Bλln M500 + Cλln E(z) and use SPT-SZ cluster masses and RM richnesses λ to constrain the parameters. We find |$B_\lambda = 1.14^{+0.21}_{-0.18}$| and |$C_\lambda =0.73^{+0.77}_{-0.75}$|⁠. The associated scatter in mass at fixed richness is |$\sigma _{\ln M|\lambda } = 0.18^{+0.08}_{-0.05}$| at a characteristic richness λ = 70. We demonstrate that our model provides an adequate description of the matched sample, showing that the fraction of SPT-SZ-selected clusters with RM counterparts is consistent with expectations and that the fraction of RM-selected clusters with SPT-SZ counterparts is in mild tension with expectation. We model the optical-SZE cluster positional offset distribution with the sum of two Gaussians, showing that it is consistent with a dominant, centrally peaked population and a subdominant population characterized by larger offsets. We also cross-match the RM catalogue with SPT-SZ candidates below the official catalogue threshold significance ξ = 4.5, using the RM catalogue to provide optical confirmation and redshifts for 15 additional clusters with ξ ∈ [4, 4.5].

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.002
metaresearch head score (Gemma)0.006
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.010
Threshold uncertainty score0.019

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.006
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0010.001
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.008
GPT teacher head0.196
Teacher spread0.188 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

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Citations131
Published2015
Admission routes1
Has abstractyes

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